Viendo archivo del viernes, 28 marzo 1997

Informe actividad solar

Any mentioned solar flare in this report has a scaling factor applied by the Space Weather Prediction Center (SWPC). Because of the SWPC scaling factor, solar flares are reported as 42% smaller than for the science quality data. The scaling factor has been removed from our archived solar flare data to reflect the true physical units.
Informe de actividad Solar-Geofísica 1997 Mar 28 2200 UTC
Preparado por NOAA © SWPC y procesado por SpaceWeatherLive.com

Informe conjunto USAF/NOAA de actividad Solar y Geofísica

SDF Número 087 Publicado el 2200Z a las 28 MAR 1997

IA. Análisis de regiones solares activas y de actividad desde 27-2100Z hasta 28-2100Z

SOLAR ACTIVITY WAS LOW. TODAY'S SOLE C-CLASS EVENT WAS CLASS C1 AT 0120Z. THERE WERE NO OBSERVATIONS AVAILABLE TO PINPOINT THE SOURCE OF THE EVENT. REGION 8026 (S24E59) IS THE ONLY SPOTTED REGION ON THE DISK AND HAS SHOWN SLOW GROWTH OVER THE PAST 24 HOURS. THE GROUP HAS NEW CYCLE POLARITY, WITH MAGNETICALLY NEGATIVE LEADERS AND POSITIVE TRAILERS.
IB. Pronóstico de la actividad solar
SOLAR ACTIVITY IS EXPECTED TO BE VERY LOW TO LOW. THERE CONTINUES TO BE A FAIR CHANCE FOR ADDITIONAL, ISOLATED C-CLASS EVENTS FROM REGION 8026.
IIA. Resumen de la actividad geofísica 27-2100Z a 28-2100Z
THE GEOMAGNETIC FIELD WAS QUIET TO UNSETTLED FROM THE BEGINNING OF THE PERIOD THROUGH ABOUT 28/1400Z, WHEN AN INCREASE IN ACTIVITY BEGAN. SINCE 1400Z, ACTIVITY RANGED FROM UNSETTLED TO MINOR STORM CONDITIONS WITH SOME ISOLATED MAJOR STORM PERIODS AT A FEW HIGH LATITUDE SITES. SOLAR WIND DATA WERE AVAILABLE BRIEFLY DURING THE DISTURBANCE AND INDICATED ENHANCED DENSITIES (10-15 P/CC), NOMINAL SPEEDS (400-430 KM/S), AND A SOUTHWARD DIRECTED INTERPLANETARY MAGNETIC FIELD OF MODERATE STRENGTH (-5 TO -10 NT). THIS SIGNATURE SUGGESTS THAT THE ACTIVITY WAS CAUSED BY A CORONAL TRANSIENT. THE GREATER THAN 2 MEV ELECTRON FLUXES WERE AT MODERATE TO HIGH LEVELS TODAY.
IIB. Pronóstico de la actividad geofísica
THE GEOMAGNETIC FIELD IS EXPECTED TO BE PREDOMINANTLY UNSETTLED FOR THE NEXT THREE DAYS.
III. Probabilidades del evento 29 MAR a 31 MAR
Clase M01%01%01%
Clase X01%01%01%
Protón01%01%01%
PCAFGREEN
IV. Penticton 10.7cm flujo
  Observado       28 MAR 073
  Previsto   29 MAR-31 MAR  074/075/076
  Media de 90 Días        28 MAR 074
V. Índices Geomagnéticos A
OBSERVED AFR/AP 27 MAR  007/006
ESTIMATED AFR/AP 28 MAR  010/010
PREDICTED AFR/AP 29 MAR-31 MAR  010/010-010/010-010/010
VI. Probabilidades de Actividad Geomagnética 29 MAR a 31 MAR
A. Latitudes Medias
Activo15%15%15%
Tormenta Menor05%05%10%
Tormenta Mayor-Severa01%01%01%
B. Latitudes Altas
Activo15%15%15%
Tormenta Menor05%05%10%
Tormenta Mayor-Severa01%01%01%

All times in UTC

< < Ir a la visión general diaria

Últimas noticias

Apoye a SpaceWeatherLive.com!

A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!

No Ads on SWL Pro!
No Ads on SWL Pro! Suscripciones
Donations
Apoye a SpaceWeatherLive.com! Donar
Apoya a SpaceWeatherLive con nuestro merchandise
Échale un ojo a nuestro merchandise

Hechos clima espacial

Último evento clase X04/02/2026X4.21
Último evento clase M16/02/2026M2.4
Últimas tormentas geomagnéticas16/02/2026Kp6 (G2)
Días sin manchas
Último día sin manchas08/06/2022
Promedio de manchas solares mensuales
enero 2026112.6 -11.4
febrero 2026103.9 -8.7
Last 30 days121.7 +18

Efemérides*

Llamarada solar
12011M9.61
22011M2.15
32011M1.97
42002M1.55
52011M1.54
DstG
11999-123G3
21961-101G3
31998-100G3
42005-80G2
52015-69G1
*desde 1994

Redes sociales